Effective two-body model for spectra of clusters of H 2, H 3, He 3, and He 4 with He 4, and H 2 - He 4 scattering
dc.contributor.author | Fraser, P. | |
dc.contributor.author | Massen-Hane, K. | |
dc.contributor.author | Kadyrov, A. | |
dc.contributor.author | Amos, K. | |
dc.contributor.author | Bray, Igor | |
dc.contributor.author | Canton, L. | |
dc.date.accessioned | 2017-08-24T02:16:38Z | |
dc.date.available | 2017-08-24T02:16:38Z | |
dc.date.created | 2017-08-24T01:43:57Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | Fraser, P. and Massen-Hane, K. and Kadyrov, A. and Amos, K. and Bray, I. and Canton, L. 2017. Effective two-body model for spectra of clusters of H 2, H 3, He 3, and He 4 with He 4, and H 2 - He 4 scattering. Physical Review C. 96 (1). | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/55119 | |
dc.identifier.doi | 10.1103/PhysRevC.96.014619 | |
dc.description.abstract |
© 2017 American Physical Society. Four light-mass nuclei are considered by an effective two-body clusterization method: Li7 as H3+He4,Be7 as He3+He4,Be8 as He4+He4, and Li6 as H2+He4. The low-energy spectra of the first three are determined from single-channel Lippmann-Schwinger equations. For the last, two uncoupled sets of equations are considered: those involving the S31 and those of the posited 1S0 states of H2. Low-energy elastic scattering cross sections are calculated from the same H2+He4 Hamiltonian, for many angles and energies for which data are available. While some of these systems may be more fully described by many-body theories, this work establishes that a large amount of data may be explained by these two-body clusterizations. | |
dc.publisher | The American Physical Society | |
dc.title | Effective two-body model for spectra of clusters of H 2, H 3, He 3, and He 4 with He 4, and H 2 - He 4 scattering | |
dc.type | Journal Article | |
dcterms.source.volume | 96 | |
dcterms.source.number | 1 | |
dcterms.source.issn | 2469-9985 | |
dcterms.source.title | Physical Review C | |
curtin.department | Department of Physics and Astronomy | |
curtin.accessStatus | Fulltext not available |
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